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A Disintegrating Rocky Planet with Prominent Comet-like Tails around a Bright Star

  • Authors: Marc Hon, Saul Rappaport, Avi Shporer, Andrew Vanderburg, Karen A. Collins, Cristilyn N. Watkins, Richard P. Schwarz, Khalid Barkaoui, Samuel W. Yee, Joshua N. Winn, Alex S. Polanski, Emily A. Gilbert, David R. Ciardi, Jeroen Audenaert, William Fong, Jack Haviland, Katharine Hesse, Daniel Muthukrishna, Glen Petitpas, Ellie Hadjiyska Schmelzer, Norio Narita, Akihiko Fukui, Sara Seager, George R. Ricker

Marc Hon et al 2025 The Astrophysical Journal Letters 984 .

  • Provider: AAS Journals

Caption: Figure 2.

(a)–(b) Light curves of BD+05 4868 A from the All-Sky Automated Survey for Supernovae (ASAS-SN) folded at a period of 1.271869 days at the ephemerides determined from TESS data. The ASAS-SN light curves are binned over 75 minute intervals. The shaded bands indicate the formal and binned flux uncertainties added in quadrature. (c) A comparison between the TESS and ASAS-SN phase-folded light curves.

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